The Borexino data-set is traditionally divided in three Phases, spaced out by hardware milestones: Phase-I, from mid-2007 to beginning of 2010, ends with the calibration campaign, in which the first measurement of the \(^{7}\) Be solar neutrino interaction rate [1]}, [2]}, [3]} has been performed; Phase-II, from the-beginning of 2012 to mid-2016, starts after an intense purification campaign, based on water extraction, with unprecedented suppression of the radioactive contaminants, in which the first evidence of the \(pep\)  neutrinos [4]} and a 10% measurement of the \(pp\)  neutrinos [5]} has been published, later updated in the solar neutrino comprehensive analysis [6]}, [7]}, [8]}; Phase-III, from mid-2016 (end of the thermal insulation installation) to October 3rd 2021 (beginning of the detector decommissioning).
In the first part of Phase-III the first detection of the CNO neutrinos [9]} has been performed. Table  summarizes the most important results concerning solar neutrinos interaction rates measured by Borexino.
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